Pith. sign in

Paper Citation Record · LEDGER

Massive black hole binary inspiral and spin evolution in a cosmological framework

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2006.06647.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2006.06647 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T05:12:17.108921Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-07T23:34:19.435306Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a93c6274-79ca-43df-a6ed-f365efdb23f7 · inbound

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations cites this paper.

Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations Massive black hole binary inspiral and spin evolution in a cosmological framework

Reference 83

Resolution
verified exact
local_arxiv, observed 2026-07-07T23:34:19.437043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:fc2f39859b8475a28e2f6ca16132c9998ca53652c3a7742db7724e2221ffa83a

Observation 1dafbfe3-0eed-4f59-ba04-803c4154d3d4 · inbound

Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook cites this paper.

Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook Massive black hole binary inspiral and spin evolution in a cosmological framework

Reference 93

Resolution
unresolved
no resolver link, observed 2026-07-31T05:12:17.108921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T05:12:17.108921Z digest=sha256:b8f5f222be2523ab0531633b8976093fa60a8b0fc9a5c077766e928fdfa82982